Some Preliminary Scientific Results of Chang’E-3 Mission

Abstract:

Chang’E-3 mission is the main task of Phase two of China Lunar Exploration Program (CLEP), and also is Chinese first probe of landing, working and roving on the moon. Chang’E-3 craft composed of a lander and a rover, and each of them carry four scientific payloads respectively. The landing site of Chang’E-3 was located at 44.12 degrees north latitude and 19.51 degrees west longitude, where is in the northern part of Imbrium Which the distance in its west direction from the landing site of former Soviet probe Luna-17 is about 400 km, and about 780km far from the landing site of Appolo-17 in its southeast direction. Unfortunately, after a series of scientific tests and exploration on the surface of the moon, the motor controller communication of the rover emerged a breakdown on January 16, 2014, which leaded the four payloads onboard the rover can’t obtain data anymore. However, we have received some interesting scientific data which have been studied by Chinese scientists. During the landing process of Chang’E-3, the Landing camera got total 4673 images with the Resolution in millimeters to meters, and the lander and rover took pictures for each other at different point with Topography camera and Panoramic camera. We can find characteristic changes in celestial brightness with time by analyzing image data from Lunar-based Ultraviolet Telescope (LUT) and an unprecedented constraint on water content in the sunlit lunar exosphere seen by LUT). The figure observed by EUV camera (EUVC) shows that there is a transient weak area of the Earth‘s plasma sphere; This event took place about three hours. The scientists think that it might be related to the change of the particle density of mid-latitude ionosphere. The preliminary spectral and mineralogical results from the landing site are derived according to the data of Visible and Near-infrared Imaging Spectrometer (VNIS). Seven major elements including Mg, Al, Si, K, Ca, Ti and Fe have been identified by the Active Particle-induced X-ay Spectrometer (APXS). The observations of Lunar Penetrating Radar (LPR) have revealed the con-figuration of regolith where the thickness of regolith varies from about 4m to 6m, and on layer of lunar rock was detected, which is about 330m deep and might have been accumulated during the depositional hiatus of mare basalts.